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Two-dimensional Core-collapse Supernova Simulations with the Isotropic Diffusion Source Approximation for Neutrino Transport
JournalArticle (Originalarbeit in einer wissenschaftlichen Zeitschrift)
 
ID 3727870
Author(s) Pan, Kuo-Chuan; Liebendörfer, Matthias; Hempel, Matthias; Thielemann, Friedrich-Karl
Author(s) at UniBasel Thielemann, Friedrich-Karl
Pan, Kuo-Chuan
Hempel, Matthias
Liebendörfer, Matthias
Year 2016
Title Two-dimensional Core-collapse Supernova Simulations with the Isotropic Diffusion Source Approximation for Neutrino Transport
Journal Astrophysical Journal
Volume 817
Number 1
Pages / Article-Number 72
Keywords hydrodynamics, instabilities, neutrinos, supernovae: general
Abstract The neutrino mechanism of core-collapse supernova is investigated via non-relativistic, two-dimensional (2D), neutrino radiation-hydrodynamic simulations. For the transport of electron flavor neutrinos, we use the interaction rates defined by Bruenn and the isotropic diffusion source approximation (IDSA) scheme, which decomposes the transported particles into trapped-particle and streaming-particle components. Heavy neutrinos are described by a leakage scheme. Unlike the “ray-by-ray” approach in some other multidimensional supernova models, we use cylindrical coordinates and solve the trapped-particle component in multiple dimensions, improving the proto-neutron star resolution and the neutrino transport in angular and temporal directions. We provide an IDSA verification by performing one-dimensional (1D) and 2D simulations with 15 and 20 M ⊙ progenitors from Woosley et al. and discuss the difference between our IDSA results and those existing in the literature. Additionally, we perform Newtonian 1D and 2D simulations from prebounce core collapse to several hundred milliseconds postbounce with 11, 15, 21, and 27 M ⊙ progenitors from Woosley et al. with the HS(DD2) equation of state. General-relativistic effects are neglected. We obtain robust explosions with diagnostic energies E dia ≳ 0.1-0.5 B (1 B ≡ 10 51 erg) for all considered 2D models within approximately 100-300 ms after bounce and find that explosions are mostly dominated by the neutrino-driven convection, although standing accretion shock instabilities are observed as well. We also find that the level of electron deleptonization during collapse dramatically affects the postbounce evolution, e.g., the neglect of neutrino-electron scattering during collapse will lead to a stronger explosion.
Publisher IOP Publishing
ISSN/ISBN 0004-637X ; 1538-4357
edoc-URL http://edoc.unibas.ch/53876/
Full Text on edoc Available
Digital Object Identifier DOI 10.3847/0004-637X/817/1/72
ISI-Number WOS:000368872400072
Document type (ISI) Article
 
   

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